SDO HMI 2014-11-01 09:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.40 | 27.11 | 5.08 | 17.40 | -17.47 | 97.83 | -33.05 | 124.97 | 0.6325 | 18.6 | -17.4 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.12 | 13.77 | 1.88 | 8.33 | -16.17 | 102.41 | -28.47 | 126.74 | 0.5735 | 995.4 | 692.8 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -15.85 | 102.35 | -28.53 | 126.22 | 0.5717 | 773.0 | 605.9 | |
| 5.28 | -1.00 | 3.20 | -1.00 | -16.21 | 102.08 | -28.79 | 126.50 | 0.5776 | 814.4 | 999999 | |
| 0.00 | 1.13 | 0.00 | 0.68 | -15.93 | 102.13 | -28.75 | 126.12 | 0.5748 | 649.0 | 574.8 | |
| 0.00 | 0.69 | 0.00 | 0.44 | -15.85 | 96.99 | -33.89 | 121.82 | 0.6336 | -515.0 | -399.2 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -18.66 | 94.02 | -36.86 | 123.53 | 0.6840 | -646.0 | -581.7 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -17.05 | 94.22 | -36.66 | 121.56 | 0.6722 | -664.0 | -631.9 | |
| 0.00 | 1.21 | 0.00 | 0.82 | -17.49 | 93.73 | -37.15 | 121.81 | 0.6802 | -527.0 | -466.9 | |
| 0.00 | 1.13 | 0.00 | 0.77 | -18.14 | 93.45 | -37.43 | 122.48 | 0.6871 | -510.0 | -373.8 | |
| 0.00 | 1.04 | 0.00 | 0.73 | -19.59 | 91.56 | -39.32 | 123.13 | 0.7152 | -478.0 | -515.4 | |
| 0.00 | 0.78 | 0.00 | 0.55 | -19.78 | 91.50 | -39.38 | 123.34 | 0.7169 | -492.0 | -437.9 | |
| 0.00 | 1.30 | 0.00 | 0.92 | -19.93 | 91.21 | -39.67 | 123.34 | 0.7207 | -542.0 | -499.7 | |
| 0.00 | 1.47 | 0.00 | 1.04 | -19.41 | 91.29 | -39.59 | 122.74 | 0.7170 | -537.0 | -356.2 | |
| 0.00 | 1.21 | 0.00 | 0.92 | -24.12 | 89.45 | -41.43 | 127.26 | 0.7611 | -246.0 | -209.4 | |
| 0.00 | 0.87 | 0.00 | 0.60 | -16.72 | 91.77 | -39.11 | 119.61 | 0.6972 | -406.0 | -465.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |